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Constraining the magnetic field geometry of the millisecond pulsar PSRJ0030+0451 from joint radio, thermal X-ray, and γ-ray emission

Pétri, J.; Guillot, S.; Guillemot, L.; Cognard, I.; Theureau, G.; Grießmeier, J. M.; Bondonneau, L.; González-Caniulef, D.; Webb, N.; Jankowski, F.; Kravtsov, I. P.; McKee, J. W.; Carozzi, T. D.; Cecconi, B.; Serylak, M.; Zarka, P.

Authors

J. Pétri

S. Guillot

L. Guillemot

I. Cognard

G. Theureau

J. M. Grießmeier

L. Bondonneau

D. González-Caniulef

N. Webb

F. Jankowski

I. P. Kravtsov

J. W. McKee

T. D. Carozzi

B. Cecconi

M. Serylak

P. Zarka



Abstract

Context. With the advent of multi-wavelength electromagnetic observations of neutron stars - spanning many decades in photon energies - from radio wavelengths up to X-rays and γ-rays, it has become possible to significantly constrain the geometry and the location of the associated emission regions. Aims. In this work, we use results from the modelling of thermal X-ray observations of PSR J0030+0451 from the Neutron Star Interior Composition Explorer (NICER) mission and phase-aligned radio and γ-ray pulse profiles to constrain the geometry of an off-centred dipole that is able to reproduce the light curves in these respective bands simultaneously. Methods. To this aim, we deduced a configuration with a simple dipole off-centred from the location of the centre of the thermal X-ray hot spots. We show that the geometry is compatible with independent constraints from radio and -ray pulsations only, leading to a fixed magnetic obliquity of α ≈ 75° and a line-of-sight inclination angle of ζ ≈ 54°. Results. We demonstrate that an off-centred dipole cannot be rejected by accounting for the thermal X-ray pulse profiles. Moreover, the crescent shape of one spot is interpreted as the consequence of a small-scale surface dipole on top of the large-scale off-centred dipole.

Citation

Pétri, J., Guillot, S., Guillemot, L., Cognard, I., Theureau, G., Grießmeier, J. M., …Zarka, P. (2023). Constraining the magnetic field geometry of the millisecond pulsar PSRJ0030+0451 from joint radio, thermal X-ray, and γ-ray emission. Astronomy and Astrophysics, 680, Article A93. https://doi.org/10.1051/0004-6361/202346913

Journal Article Type Article
Acceptance Date Sep 5, 2023
Online Publication Date Dec 15, 2023
Publication Date Dec 1, 2023
Deposit Date Jan 8, 2024
Publicly Available Date Jan 9, 2024
Journal Astronomy and Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 680
Article Number A93
DOI https://doi.org/10.1051/0004-6361/202346913
Keywords stars: neutron; pulsars: individual: PSR J0030+0451; stars: rotation; magnetic fields; gamma rays: stars; X-rays: stars
Public URL https://hull-repository.worktribe.com/output/4501029

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0

Copyright Statement
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.




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